Publications
Publications from 2004 to present can be accessed through ADS at this link. Older publications are listed below.
Shantanu Basu & C. E. Jones, On the Power-Law Tail in the Mass Function of Protostellar Condensations and Stars, 2004,
Mon. Not. R. Astron. Soc., vol. 347, issue 3, page L47-L51. Preprints: postscript file
, or pdf file.
A. Lenorzer, A. Bik, A. de Koter, S. E. Kurtz, L.B.F.M. Waters, L. Kaper, C. E. Jones, & T. R. Geballe
2004,
The peculiar circumstellar environment of NGC2024-IRS2 ,
Astronomy and Astrophysics, 414, 245.
C. R. Kerton, Christopher M. Brunt, C. E. Jones, & Shantanu Basu 2003,
On the intrinsic shape of
molecular clouds, Astronomy and Astrophysics, 411,149.
C. E. Jones & Shantanu Basu, The Intrinsic Shapes of Molecular Cloud
Fragments over a Range of Length Scales, paper with
colored figures , or paper with gray-scale
figures . This paper is published in ApJ April 10, 2002, 569, 280. (If you are printing in black and white,
retrieve the paper with the gray-scale figures so that there are no ambiguities
with the color scale in the shaded graphs.)
C. E. Jones, Shantanu Basu, & John Dubinski,
Intrinsic Shapes of Molecular Cloud Cores. In this paper we
investigate axisymmetric oblate and prolate molecular cloud cores via
an analytical method. We show that both oblate and prolate
axisymmetric cores lead to results which are unphysical. We
demonstrate statistically, that intrinsic triaxial cores produce
projected distributions which compare well with observations. This
paper is published in ApJ 2001, 551:387.
C. E. Millar, T. A. A. Sigut & J. M. Marlborough,
The Continuum Re-processing Efficiency of Be Star Circumstellar Disks,
MNRAS 2000, 312,465. We have calculated the total flux emitted in H alpha,
P alpha, and Br alpha by the
circumstellar envelope of both an early Be star, gamma Cas, and a late
Be star, 1 Delphini, assuming the central star is the
only source of energy input into the circumstellar envelope. We find
that an additional source of ionizing photons is not necessary to
account for the observed emission.
S. Hony, L. B. F. M. Waters, P. A. Zaal, A. de Koter, J. M.Marlborough, C. E. Millar, N. R. Trams, P. W. Morris, & Th. de Graauw,
The infrared spectrum of the Be star gamma Cassiopeiae , A&A 2000, 355, 187
C. E. Millar, T. A. A. Sigut, and J. M. Marlborough,
Rates of Energy Gain and Loss in the Circumstellar Envelopes
of Be Stars . In this article, we demonstrate that a single
central B star
produces sufficient photoionizing radiation to fully account for
observed Halpha fluxes. This is in disagreement with the results of
K. M. V. Apparao, Be Star
Newsletter, Vol 33, who argues that an additional source of
photoionizing radiation is necessary for the later type Be stars.
Our article appears in the
current issue of the
Be Star
Newsletter, Vol 34.
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